The Cardy-Verlinde Formula and Asymptotically de Sitter Brane Universe

Simple item page
dc.creatorYoum, Donam
dc.date2001-11-29
dc.date2002-02-25
dc.date.accessioned2026-07-07T04:12:46Z
dc.date.available2026-07-07T04:12:46Z
dc.descriptionWe consider the brane universe in the bulk background of the topological AdS-Schwarzschild black holes, where the brane tension takes larger value than the fine-tunned value. The resulting universe is radiation dominated and has positive cosmological constant. We obtain the associated cosmological Cardy formula and the Cardy-Verlinde formula. We also derive the Hubble and the Bekenstein entropy bounds from the conjectured holography bound on the Casimir entropy.
dc.description12 pages, LaTeX, revised version with minor corrections to appear in Phys. Lett. B
dc.identifierhttps://arxiv.org/abs/hep-th/0111276
dc.identifierhttp://arxiv.org/abs/hep-th/0111276
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51023
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe Cardy-Verlinde Formula and Asymptotically de Sitter Brane Universe
dc.typetext

Files

Collections

arXiv